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ANALYSIS OF SOLAR PLASMA DYNAMICS DURING A CORONAL MASS EJECTION FROM THE SUN USING THE PIVLAB SOFTWARE
- Authors: Kalamanov V.G.1, Sadovsky A.M.1
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Affiliations:
- Space Research Institute, Russian Academy of Sciences
- Issue: Vol 51, No 9 (2025)
- Pages: 983-989
- Section: SPACE PLASMA
- URL: https://journal-vniispk.ru/0367-2921/article/view/382346
- DOI: https://doi.org/10.31857/S0367292125090046
- ID: 382346
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Abstract
The possibility of using the PIV (particle image velocimetry) method as an alternative to the existing methods used to analyze the dynamics of solar plasma during a coronal mass ejection is considered. PIVLab software was used to perform a comprehensive analysis of a coronal mass ejection dynamics. The linear speed and the velocity field of the coronal mass ejection were calculated. The study showed that the software is capable of measuring changes in the coronal structure and record the processes that lead to the observed changes.
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About the authors
V. G. Kalamanov
Space Research Institute, Russian Academy of Sciences
Email: VGKalamanov@cosmos.ru
Moscow, Russia
A. M. Sadovsky
Space Research Institute, Russian Academy of SciencesMoscow, Russia
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